Black holes behave as thermodynamic objects with a Bekenstein-Hawking entropy and a Hawking temperature [1]}, [2]}, [3]}, [4]}, [5]}, [6]}, [7]}, and set deep connection between the laws of classical general relativity, thermodynamics, and quantum mechanics due to the presence of
horizons [1]}, [2]}, [3]}, [4]}, [5]}, [6]}, [7]}, [15]}, [16]}, [17]}. It is suggested that black holes have very massive entropy in the universe, i.e., their entropies are greater than any other object of the same volume [4]}, [6]}. This entropy is defined by \(S = A/4\) . However, it is found that quantum fluctuations on the planck scale may change the entropy of the black holes with time. These quantum fluctuations become important when the black hole shrinks its size and therefore, entropy of the black holes need to get corrected. In order to get corrections on the black hole entropy different approaches such as non-perturbative quantum general relativity, the Cardy formula, the exact partition function, matter fields in backgrounds of a black hole, Rademacher expansion of the partition function and string theoretical effects have been used [20]}, [21]}, [22]}, [23]}, [24]}, [25]}, [26]}, [27]}, [28]}, [29]}, [30]}, [31]}. On the other hand, recently the corrections to the black hole entropy can be obtained through the the generalized uncertainty principle [32]}, [33]}, [34]}.
